J/MNRAS/485/3623  Red giants abundance analysis in open clusters  (Reddy+, 2019)

Comprehensive abundance analysis of red giants in the open clusters Stock 2, NGC 2168, 6475, 6991, and 7762. Reddy A.B.S., Lambert D.L. <Mon. Not. R. Astron. Soc., 485, 3623-3641 (2019)> =2019MNRAS.485.3623R 2019MNRAS.485.3623R (SIMBAD/NED BibCode)
ADC_Keywords: Abundances ; Clusters, open ; Spectra, optical ; Effective temperatures ; Positional data ; Stars, giant Keywords: stars: abundances - Galaxy: abundances - Galaxy: disc - Galaxy: kinematics and dynamics - open clusters and associations: general - open clusters and associations: individual: Stock 2, NGC 2168, NGC 6475, NGC 6991 and NGC 7762 Abstract: We have analysed high-dispersion Echelle spectra (R=60000) of red giant members of five open clusters to derive abundances for many elements from Na to Eu. The [Fe/H] values are -0.06±0.03 for Stock 2, -0.11±0.03 for NGC 2168, -0.01±0.03 for NGC 6475, 0.00±0.03 for NGC 6991, and -0.07±0.03 for NGC 7662. Sodium is enriched in the giants relative to the abundance expected of main-sequence stars of the same metallicity. This enrichment of [Na/Fe] by about +0.25 attributed to the first dredge-up is discussed in the light of theoretical predictions and recently published abundance determinations. Abundance ratios [El/Fe] for other elements are with very few exceptions equal to those of field giants and dwarfs, i.e. [El/Fe]∼0.00 for [Fe/H]∼0.0. An exception is the overabundance of La, Ce, Nd, and Sm in NGC 6991 but this is consistent with our previous demonstration that the abundances of these s-process products vary by about ±0.2 among clusters of the same [Fe/H], a variation found also among field giants and dwarfs. Description: Selection of red giants for subsequent spectroscopic observations was made by identifying stars having common proper motions at the putative red giant clump in the cluster colour-magnitude diagram (CMD). The CMDs were created from the available BV and Gaia DR2 photometric magnitudes. High-resolution and high signal-to-noise (S/N) ratio optical spectra of 18 giant stars in six OCs, namely Stock 2 (3 giants), NGC 2168 (3 giants), NGC 6475 (3 giants), NGC 6991 (4 giants), and NGC 7762 (3 giants) were observed in 2016 September, October, and November with the Robert G. Tull coude cross-dispersed Echelle spectrograph (Tull et al. 1995PASP..107..251T 1995PASP..107..251T) at the 2.7-m Harlan J. Smith Telescope of the McDonald Observatory. On all occasions we employed the camera with a 2048x2048 24µm pixel CCD detector and 52.67 grooves/mm Echelle grating with exposures centred at 5060Å in order 69. We secured two to four exposures of cluster giants in our target list (Table 1) with each exposure limited to 20-30min to minimize the influence of cosmic rays and to acquire a global S/N of above 100. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 98 18 The journal of the observations for the cluster members table2.dat 65 18 Photometric and spectroscopic atmospheric parameters for open cluster members analysed in this study table3.dat 316 5 Elemental abundance ratios [El/Fe] for elements from Na to Eu for Stock 2, NGC 2168, 6475, 6991, and 7762 from this study table4.dat 54 5 Cluster fundamental parameters derived in this study using the BV and Gaia-based CMDs table5.dat 103 5 Cluster fundamental parameters derived by taking the mean of Gaia astrometric parameters of cluster members table6.dat 384 4 The chemical abundances of red giants (ID: 43, 1011, 1082) in the star cluster Stock 2 table7.dat 396 7 The chemical abundances of stars (IDs: 81, 310, and 662) in NGC 2168 and stars (IDs: 134 and HD 162496) in NGC 6475 table8.dat 387 5 The chemical abundances of stars (IDs: 22, 67, 100, and 131) in NGC 6991 table9.dat 369 4 The chemical abundances of stars (IDs: 35, 91, and 110) in NGC 7762 table10.dat 66 31 Mean LTE and non-LTE abundances of Na and Al in OCs analysed in this paper and in Reddy et al. (2012MNRAS.419.1350R 2012MNRAS.419.1350R, Cat. J/MNRAS/419/1350, 2013MNRAS.431.3338R 2013MNRAS.431.3338R, Cat. J/MNRAS/431/3338, 2015MNRAS.450.4301R 2015MNRAS.450.4301R, Cat. J/MNRAS/450/4301, 2016MNRAS.463.4366R 2016MNRAS.463.4366R) -------------------------------------------------------------------------------- See also: I/345 : Gaia DR2 (Gaia Collaboration, 2018) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Cluster Cluster name 10- 18 A9 --- Star Star ID 20 I1 --- f_Star ? Flag on Star (1) 22- 23 I2 h RAh Right ascension (J2000) 25- 26 I2 min RAm Right ascension (J2000) 28- 32 F5.2 s RAs Right ascension (J2000) 34 A1 --- DE- Declination sign (J2000) 35- 36 I2 deg DEd Declination (J2000) 38- 39 I2 arcmin DEm Declination (J2000) 41- 45 F5.2 arcsec DEs Declination (J2000) 47- 51 F5.2 mag Vmag ? V magnitude 53- 56 F4.2 mag B-V ? B-V colour index 58- 61 F4.2 mag V-Ks ? V-Ks colour index 63- 66 F4.2 mag J-Ks ? J-Ks colour index 68- 72 F5.1 km/s RV Radial heliocentric velocity 74- 76 F3.1 km/s e_RV Error on RV 78- 80 I3 --- S/N Signal to noise ratio 82- 91 I10 "Y:M:D" Date Observation date 93- 98 A6 --- Exp Exposure time -------------------------------------------------------------------------------- Note (1): Flag as follows: 1 = First component of the observed spectrum of HD 162587 2 = Second component of the observed spectrum of HD 162587 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Cluster Cluster name 10- 18 A9 --- Star Star ID 20 I1 --- f_Star ? Flag on Star (1) 22- 25 I4 K TeffBV ? Effective temperature deduced from B-V (2) 27- 30 I4 K TeffVK ? Effective temperature deduced from V-K (2) 32- 35 I4 K TeffJK ? Effective temperature deduced from J-K (2) 37- 40 F4.2 [cm/s2] loggph ? Photometric estimate of surface gravity (3) 42- 45 I4 K Teffsp ? Spectroscopic effective temperature 47- 50 F4.2 [cm/s2] loggsp ? Spectroscopic surface gravity 52- 55 F4.2 km/s vturbsp ? Microturbulence velocity 57- 60 F4.2 [Lsun] logLph ? log of photometric stellar luminosity 62- 65 F4.2 [Lsun] logLsp ? log of spectroscopic stellar luminosity -------------------------------------------------------------------------------- Note (1): Flag as follows: 1 = First component of the observed spectrum of HD 162587 2 = Second component of the observed spectrum of HD 162587 Note (2): We derived the star's photometric effective temperature, by substituting the dereddened photometric colours into the infrared flux method based colour-temperature calibrations of Alonso, Arribas & Martinez-Roger (1999A&AS..140..261A 1999A&AS..140..261A). Note (3): The photometric estimates of surface gravities, were made by incorporating the heliocentric distance of the cluster, photometric temperature, bolometric correction, cluster turn-off mass, and the solar parameters of Teff=5777K and logg =4.44cm/s2 into the well-known logg-Teff relation (Reddy et al. 2012MNRAS.419.1350R 2012MNRAS.419.1350R, Cat. J/MNRAS/419/1350). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Cluster Cluster name 10- 13 F4.2 [-] [NaI/Fe] NaI to iron abundance ratio 15- 18 F4.2 [-] e_[NaI/Fe] Error on [NaI/Fe] 20- 24 F5.2 [-] [MgI/Fe] MgI to iron abundance ratio 26- 29 F4.2 [-] e_[MgI/Fe] Error on [MgI/Fe] 31- 34 F4.2 [-] [AlI/Fe] AlI to iron abundance ratio 36- 39 F4.2 [-] e_[AlI/Fe] Error on [AlI/Fe] 41- 44 F4.2 [-] [SiI/Fe] SiI to iron abundance ratio 46- 49 F4.2 [-] e_[SiI/Fe] Error on [SiI/Fe] 51- 55 F5.2 [-] [CaI/Fe] CaI to iron abundance ratio 57- 60 F4.2 [-] e_[CaI/Fe] Error on [CaI/Fe] 62- 65 F4.2 [-] [ScI/Fe] ? ScI to iron abundance ratio 67- 70 F4.2 [-] e_[ScI/Fe] ? Error on [ScI/Fe] 72- 76 F5.2 [-] [ScII/Fe] ScII to iron abundance ratio 78- 81 F4.2 [-] e_[ScII/Fe] Error on [ScII/Fe] 83- 87 F5.2 [-] [ScII/Fe]s ScII to iron abundance ratio calculated by synthesis 89- 92 F4.2 [-] e_[ScII/Fe]s Error on [ScII/Fe]s 94- 98 F5.2 [-] [TiI/Fe] TiI to iron abundance ratio 100-103 F4.2 [-] e_[TiI/Fe] Error on [TiI/Fe] 105-109 F5.2 [-] [TiII/Fe] TiII to iron abundance ratio 111-114 F4.2 [-] e_[TiII/Fe] Error on [TiII/Fe] 116-120 F5.2 [-] [VI/Fe] VI to iron abundance ratio 122-125 F4.2 [-] e_[VI/Fe] Error on [VI/Fe] 127-131 F5.2 [-] [CrI/Fe] CrI to iron abundance ratio 133-136 F4.2 [-] e_[CrI/Fe] Error on [CrI/Fe] 138-141 F4.2 [-] [CrII/Fe] CrII to iron abundance ratio 143-146 F4.2 [-] e_[CrII/Fe] Error on [CrII/Fe] 148-152 F5.2 [-] [MnI/Fe] MnI to iron abundance ratio calculated by synthesis 154-157 F4.2 [-] e_[MnI/Fe] Error on [MnI/Fe] 159-163 F5.2 [-] [FeI/H] FeI to hydrogen abundance ratio 165-168 F4.2 [-] e_[FeI/H] Error on [FeI/H] 170-174 F5.2 [-] [FeII/H] FeII to hydrogen abundance ratio 176-179 F4.2 [-] e_[FeII/H] Error on [FeII/H] 181-185 F5.2 [-] [CoI/Fe] CoI to iron abundance ratio 187-190 F4.2 [-] e_[CoI/Fe] Error on [CoI/Fe] 192-196 F5.2 [-] [NiI/Fe] NiI to iron abundance ratio 198-201 F4.2 [-] e_[NiI/Fe] Error on [NiI/Fe] 203-207 F5.2 [-] [CuI/Fe] CuI to iron abundance ratio calculated by synthesis 209-212 F4.2 [-] e_[CuI/Fe] Error on [CuI/Fe] 214-218 F5.2 [-] [ZnI/Fe] ZnI to iron abundance ratio calculated by synthesis 220-223 F4.2 [-] e_[ZnI/Fe] Error on [ZnI/Fe] 225-229 F5.2 [-] [YII/Fe] YII to iron abundance ratio 231-234 F4.2 [-] e_[YII/Fe] Error on [YII/Fe] 236-240 F5.2 [-] [ZrI/Fe] ZrI to iron abundance ratio 242-245 F4.2 [-] e_[ZrI/Fe] Error on [ZrI/Fe] 247-250 F4.2 [-] [ZrII/Fe] ZrII to iron abundance ratio 252-255 F4.2 [-] e_[ZrII/Fe] Error on [ZrII/Fe] 257-260 F4.2 [-] [BaII/Fe] BaII to iron abundance ratio calculated by synthesis 262-265 F4.2 [-] e_[BaII/Fe] Error on [BaII/Fe] 267-271 F5.2 [-] [LaII/Fe] LaII to iron abundance ratio 273-276 F4.2 [-] e_[LaII/Fe] Error on [LaII/Fe] 278-281 F4.2 [-] [CeII/Fe] CeII to iron abundance ratio 283-286 F4.2 [-] e_[CeII/Fe] Error on [CeII/Fe] 288-291 F4.2 [-] [NdII/Fe] NdII to iron abundance ratio 293-296 F4.2 [-] e_[NdII/Fe] Error on [NdII/Fe] 298-301 F4.2 [-] [SmII/Fe] SmII to iron abundance ratio 303-306 F4.2 [-] e_[SmII/Fe] Error on [SmII/Fe] 308-311 F4.2 [-] [EuII/Fe] EuII to iron abundance ratio calculated by synthesis 313-316 F4.2 [-] e_[EuII/Fe] Error on [EuII/Fe] -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Cluster Cluster name 10- 14 F5.2 [-] [Fe/H] Iron to hydrogen abundance ratio 16- 19 F4.2 mag E(B-V) Reddening 21- 25 F5.2 mag DMV Distance modulus V-Mv 27- 30 I4 Myr AgeBV Age using (V,B-V) colour-magnitude diagram 32- 34 I3 pc dBV Distance using (V,B-V) colour-magnitude diagram 36- 39 F4.2 mag E(BP-RP) Reddening using Gaia DR2 BP and RP magnitudes (1) 41- 45 F5.2 mag DMG Distance modulus using Gaia DR2 photometry (1) 47- 49 I3 pc dG Distance using colour-magnitude diagrams based on Gaia DR2 photometry (1) 51- 54 I4 Myr AgeG Age using colour-magnitude diagrams based on Gaia DR2 photometry (1) -------------------------------------------------------------------------------- Note (1): Values computed using Gaia DR2 photometry (Gaia Collaboration 2018A&A...616A...1G 2018A&A...616A...1G, Cat. I/345) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Cluster Cluster name 10- 12 I3 pc d Mean distance of all cluster members 14- 16 I3 pc E_d Upper error on d 18- 19 I2 pc e_d Lower error on d 21- 24 F4.2 mas plx Mean parallax of all cluster members 26- 29 F4.2 mas e_plx Error on plx 31- 36 F6.3 mas/yr pmRA Mean proper motion in right ascension of all cluster members 38- 42 F5.3 mas/yr e_pmRA Error on pmRA 44- 50 F7.3 mas/yr pmDE Mean proper motion in declination of all cluster members 52- 56 F5.3 mas/yr e_pmDE Error on pmDE 58- 60 I3 pc dRG Mean distance of the red giants analysed in this paper 62- 63 I2 pc E_dRG Upper error on dRG 65- 66 I2 pc e_dRG Lower error on dRG 68- 71 F4.2 mas plxRG Mean parallax of the red giants analysed in this paper 73- 76 F4.2 mas e_plxRG Error on plxRG 78- 83 F6.3 mas/yr pmRARG Mean proper motion in right ascension of the red giants analysed in this paper 85- 89 F5.3 mas/yr e_pmRARG Error on pmRARG 91- 97 F7.3 mas/yr pmDERG Mean proper motion in declination of the red giants analysed in this paper 99-103 F5.3 mas/yr e_pmDERG Error on pmDERG -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- Cluster Cluster name 9- 12 A4 --- Star Star ID (Avg stands for the average of the entire cluster) 14- 17 F4.2 [-] [NaI/Fe] NaI to iron abundance ratio 19- 22 F4.2 [-] e_[NaI/Fe] Error on [NaI/Fe] 24 I1 --- o_[NaI/Fe] ? Number of lines used to calculate [NaI/Fe] 26- 29 F4.2 [-] [MgI/Fe] MgI to iron abundance ratio 31- 34 F4.2 [-] e_[MgI/Fe] Error on [MgI/Fe] 36 I1 --- o_[MgI/Fe] ? Number of lines used to calculate [MgI/Fe] 38- 41 F4.2 [-] [AlI/Fe] AlI to iron abundance ratio 43- 46 F4.2 [-] e_[AlI/Fe] Error on [AlI/Fe] 48 I1 --- o_[AlI/Fe] ? Number of lines used to calculate [AlI/Fe] 50- 53 F4.2 [-] [SiI/Fe] SiI to iron abundance ratio 55- 58 F4.2 [-] e_[SiI/Fe] Error on [SiI/Fe] 60- 61 I2 --- o_[SiI/Fe] ? Number of lines used to calculate [SiI/Fe] 63- 67 F5.2 [-] [CaI/Fe] CaI to iron abundance ratio 69- 72 F4.2 [-] e_[CaI/Fe] Error on [CaI/Fe] 74- 75 I2 --- o_[CaI/Fe] ? Number of lines used to calculate [CaI/Fe] 77- 80 F4.2 [-] [ScI/Fe] ? ScI to iron abundance ratio 82- 85 F4.2 [-] e_[ScI/Fe] ? Error on [ScI/Fe] 87 I1 --- o_[ScI/Fe] ? Number of lines used to calculate [ScI/Fe] 89- 92 F4.2 [-] [ScII/Fe] ScII to iron abundance ratio 94- 97 F4.2 [-] e_[ScII/Fe] Error on [ScII/Fe] 99 I1 --- o_[ScII/Fe] ? Number of lines used to calculate [ScII/Fe] 101-104 F4.2 [-] [ScII/Fe]s ScII to iron abundance ratio calculated by synthesis 106-109 F4.2 [-] e_[ScII/Fe]s Error on [ScII/Fe]s 111 I1 --- o_[ScII/Fe]s ? Number of lines used to calculate [ScII/Fe]s 113-117 F5.2 [-] [TiI/Fe] TiI to iron abundance ratio 119-122 F4.2 [-] e_[TiI/Fe] Error on [TiI/Fe] 124-125 I2 --- o_[TiI/Fe] ? Number of lines used to calculate [TiI/Fe] 127-131 F5.2 [-] [TiII/Fe] TiII to iron abundance ratio 133-136 F4.2 [-] e_[TiII/Fe] Error on [TiII/Fe] 138 I1 --- o_[TiII/Fe] ? Number of lines used to calculate [TiII/Fe] 140-144 F5.2 [-] [VI/Fe] VI to iron abundance ratio 146-149 F4.2 [-] e_[VI/Fe] Error on [VI/Fe] 151-152 I2 --- o_[VI/Fe] ? Number of lines used to calculate [VI/Fe] 154-158 F5.2 [-] [CrI/Fe] CrI to iron abundance ratio 160-163 F4.2 [-] e_[CrI/Fe] Error on [CrI/Fe] 165 I1 --- o_[CrI/Fe] ? Number of lines used to calculate [CrI/Fe] 167-170 F4.2 [-] [CrII/Fe] CrII to iron abundance ratio 172-175 F4.2 [-] e_[CrII/Fe] Error on [CrII/Fe] 177 I1 --- o_[CrII/Fe] ? Number of lines used to calculate [CrII/Fe] 179-183 F5.2 [-] [MnI/Fe] MnI to iron abundance ratio calculated by synthesis 185-188 F4.2 [-] e_[MnI/Fe] Error on [MnI/Fe] 190 I1 --- o_[MnI/Fe] ? Number of lines used to calculate [MnI/Fe] 192-196 F5.2 [-] [FeI/H] FeI to hydrogen abundance ratio 198-201 F4.2 [-] e_[FeI/H] Error on [FeI/H] 203-205 I3 --- o_[FeI/H] ? Number of lines used to calculate [FeI/H] 207-211 F5.2 [-] [FeII/H] FeII to hydrogen abundance ratio 213-216 F4.2 [-] e_[FeII/H] Error on [FeII/H] 218-219 I2 --- o_[FeII/H] ? Number of lines used to calculate [FeII/H] 221-225 F5.2 [-] [CoI/Fe] CoI to iron abundance ratio 227-230 F4.2 [-] e_[CoI/Fe] Error on [CoI/Fe] 232 I1 --- o_[CoI/Fe] ? Number of lines used to calculate [CoI/Fe] 234-238 F5.2 [-] [NiI/Fe] NiI to iron abundance ratio 240-243 F4.2 [-] e_[NiI/Fe] Error on [NiI/Fe] 245-246 I2 --- o_[NiI/Fe] ? Number of lines used to calculate [NiI/Fe] 248-252 F5.2 [-] [CuI/Fe] CuI to iron abundance ratio calculated by synthesis 254-257 F4.2 [-] e_[CuI/Fe] Error on [CuI/Fe] 259 I1 --- o_[CuI/Fe] ? Number of lines used to calculate [CuI/Fe] 261-265 F5.2 [-] [ZnI/Fe] ZnI to iron abundance ratio calculated by synthesis 267-270 F4.2 [-] e_[ZnI/Fe] Error on [ZnI/Fe] 272 I1 --- o_[ZnI/Fe] ? Number of lines used to calculate [ZnI/Fe] 274-278 F5.2 [-] [YII/Fe] YII to iron abundance ratio 280-283 F4.2 [-] e_[YII/Fe] Error on [YII/Fe] 285-286 I2 --- o_[YII/Fe] ? Number of lines used to calculate [YII/Fe] 288-291 F4.2 [-] [ZrI/Fe] ZrI to iron abundance ratio 293-296 F4.2 [-] e_[ZrI/Fe] Error on [ZrI/Fe] 298 I1 --- o_[ZrI/Fe] ? Number of lines used to calculate [ZrI/Fe] 300-303 F4.2 [-] [ZrII/Fe] ZrII to iron abundance ratio 305-308 F4.2 [-] e_[ZrII/Fe] Error on [ZrII/Fe] 310 I1 --- o_[ZrII/Fe] ? Number of lines used to calculate [ZrII/Fe] 312-315 F4.2 [-] [BaII/Fe] BaII to iron abundance ratio calculated by synthesis 317-320 F4.2 [-] e_[BaII/Fe] Error on [BaII/Fe] 322 I1 --- o_[BaII/Fe] ? Number of lines used to calculate [BaII/Fe] 324-328 F5.2 [-] [LaII/Fe] LaII to iron abundance ratio 330-333 F4.2 [-] e_[LaII/Fe] Error on [LaII/Fe] 335 I1 --- o_[LaII/Fe] ? Number of lines used to calculate [LaII/Fe] 337-340 F4.2 [-] [CeII/Fe] CeII to iron abundance ratio 342-345 F4.2 [-] e_[CeII/Fe] Error on [CeII/Fe] 347 I1 --- o_[CeII/Fe] ? Number of lines used to calculate [CeII/Fe] 349-352 F4.2 [-] [NdII/Fe] NdII to iron abundance ratio 354-357 F4.2 [-] e_[NdII/Fe] Error on [NdII/Fe] 359-360 I2 --- o_[NdII/Fe] ? Number of lines used to calculate [NdII/Fe] 362-365 F4.2 [-] [SmII/Fe] SmII to iron abundance ratio 367-370 F4.2 [-] e_[SmII/Fe] Error on [SmII/Fe] 372 I1 --- o_[SmII/Fe] ? Number of lines used to calculate [SmII/Fe] 374-377 F4.2 [-] [EuII/Fe] EuII to iron abundance ratio calculated by synthesis 379-382 F4.2 [-] e_[EuII/Fe] Error on [EuII/Fe] 384 I1 --- o_[EuII/Fe] ? Number of lines used to calculate [EuII/Fe] -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Cluster Cluster name 10- 18 A9 --- Star Star ID (Avg stands for the average of the entire cluster) 20- 23 F4.2 [-] [NaI/Fe] NaI to iron abundance ratio 25- 28 F4.2 [-] e_[NaI/Fe] Error on [NaI/Fe] 30 I1 --- o_[NaI/Fe] ? Number of lines used to calculate [NaI/Fe] 32- 35 F4.2 [-] [MgI/Fe] MgI to iron abundance ratio 37- 40 F4.2 [-] e_[MgI/Fe] Error on [MgI/Fe] 42 I1 --- o_[MgI/Fe] ? Number of lines used to calculate [MgI/Fe] 44- 47 F4.2 [-] [AlI/Fe] AlI to iron abundance ratio 49- 52 F4.2 [-] e_[AlI/Fe] Error on [AlI/Fe] 54 I1 --- o_[AlI/Fe] ? Number of lines used to calculate [AlI/Fe] 56- 59 F4.2 [-] [SiI/Fe] SiI to iron abundance ratio 61- 64 F4.2 [-] e_[SiI/Fe] Error on [SiI/Fe] 66- 67 I2 --- o_[SiI/Fe] ? Number of lines used to calculate [SiI/Fe] 69- 73 F5.2 [-] [CaI/Fe] CaI to iron abundance ratio 75- 78 F4.2 [-] e_[CaI/Fe] Error on [CaI/Fe] 80- 81 I2 --- o_[CaI/Fe] ? Number of lines used to calculate [CaI/Fe] 83- 87 F5.2 [-] [ScI/Fe] ? ScI to iron abundance ratio 89- 92 F4.2 [-] e_[ScI/Fe] ? Error on [ScI/Fe] 94 I1 --- o_[ScI/Fe] ? Number of lines used to calculate [ScI/Fe] 96-100 F5.2 [-] [ScII/Fe] ScII to iron abundance ratio 102-105 F4.2 [-] e_[ScII/Fe] Error on [ScII/Fe] 107 I1 --- o_[ScII/Fe] ? Number of lines used to calculate [ScII/Fe] 109-113 F5.2 [-] [ScII/Fe]s ScII to iron abundance ratio calculated by synthesis 115-118 F4.2 [-] e_[ScII/Fe]s Error on [ScII/Fe]s 120 I1 --- o_[ScII/Fe]s ? Number of lines used to calculate [ScII/Fe]s 122-126 F5.2 [-] [TiI/Fe] TiI to iron abundance ratio 128-131 F4.2 [-] e_[TiI/Fe] Error on [TiI/Fe] 133-134 I2 --- o_[TiI/Fe] ? Number of lines used to calculate [TiI/Fe] 136-140 F5.2 [-] [TiII/Fe] TiII to iron abundance ratio 142-145 F4.2 [-] e_[TiII/Fe] Error on [TiII/Fe] 147 I1 --- o_[TiII/Fe] ? Number of lines used to calculate [TiII/Fe] 149-153 F5.2 [-] [VI/Fe] VI to iron abundance ratio 155-158 F4.2 [-] e_[VI/Fe] Error on [VI/Fe] 160-161 I2 --- o_[VI/Fe] ? Number of lines used to calculate [VI/Fe] 163-167 F5.2 [-] [CrI/Fe] CrI to iron abundance ratio 169-172 F4.2 [-] e_[CrI/Fe] Error on [CrI/Fe] 174 I1 --- o_[CrI/Fe] ? Number of lines used to calculate [CrI/Fe] 176-180 F5.2 [-] [CrII/Fe] CrII to iron abundance ratio 182-185 F4.2 [-] e_[CrII/Fe] Error on [CrII/Fe] 187 I1 --- o_[CrII/Fe] ? Number of lines used to calculate [CrII/Fe] 189-193 F5.2 [-] [MnI/Fe] MnI to iron abundance ratio calculated by synthesis 195-198 F4.2 [-] e_[MnI/Fe] Error on [MnI/Fe] 200 I1 --- o_[MnI/Fe] ? Number of lines used to calculate [MnI/Fe] 202-206 F5.2 [-] [FeI/H] FeI to hydrogen abundance ratio 208-211 F4.2 [-] e_[FeI/H] Error on [FeI/H] 213-215 I3 --- o_[FeI/H] ? Number of lines used to calculate [FeI/H] 217-221 F5.2 [-] [FeII/H] FeII to hydrogen abundance ratio 223-226 F4.2 [-] e_[FeII/H] Error on [FeII/H] 228-229 I2 --- o_[FeII/H] ? Number of lines used to calculate [FeII/H] 231-234 F4.2 [-] [CoI/Fe] CoI to iron abundance ratio 236-239 F4.2 [-] e_[CoI/Fe] Error on [CoI/Fe] 241 I1 --- o_[CoI/Fe] ? Number of lines used to calculate [CoI/Fe] 243-247 F5.2 [-] [NiI/Fe] NiI to iron abundance ratio 249-252 F4.2 [-] e_[NiI/Fe] Error on [NiI/Fe] 254-255 I2 --- o_[NiI/Fe] ? Number of lines used to calculate [NiI/Fe] 257-261 F5.2 [-] [CuI/Fe] CuI to iron abundance ratio calculated by synthesis 263-266 F4.2 [-] e_[CuI/Fe] Error on [CuI/Fe] 268 I1 --- o_[CuI/Fe] ? Number of lines used to calculate [CuI/Fe] 270-274 F5.2 [-] [ZnI/Fe] ZnI to iron abundance ratio calculated by synthesis 276-279 F4.2 [-] e_[ZnI/Fe] Error on [ZnI/Fe] 281 I1 --- o_[ZnI/Fe] ? Number of lines used to calculate [ZnI/Fe] 283-287 F5.2 [-] [YII/Fe] YII to iron abundance ratio 289-292 F4.2 [-] e_[YII/Fe] Error on [YII/Fe] 294-295 I2 --- o_[YII/Fe] ? Number of lines used to calculate [YII/Fe] 297-301 F5.2 [-] [ZrI/Fe] ZrI to iron abundance ratio 303-306 F4.2 [-] e_[ZrI/Fe] Error on [ZrI/Fe] 308 I1 --- o_[ZrI/Fe] ? Number of lines used to calculate [ZrI/Fe] 310-313 F4.2 [-] [ZrII/Fe] ZrII to iron abundance ratio 315-318 F4.2 [-] e_[ZrII/Fe] Error on [ZrII/Fe] 320 I1 --- o_[ZrII/Fe] ? Number of lines used to calculate [ZrII/Fe] 322-325 F4.2 [-] [BaII/Fe] BaII to iron abundance ratio calculated by synthesis 327-330 F4.2 [-] e_[BaII/Fe] Error on [BaII/Fe] 332 I1 --- o_[BaII/Fe] ? Number of lines used to calculate [BaII/Fe] 334 A1 --- f_[BaII/Fe] Flag on [BaII/Fe] (1) 336-340 F5.2 [-] [LaII/Fe] LaII to iron abundance ratio 342-345 F4.2 [-] e_[LaII/Fe] Error on [LaII/Fe] 347 I1 --- o_[LaII/Fe] ? Number of lines used to calculate [LaII/Fe] 349-353 F5.2 [-] [CeII/Fe] CeII to iron abundance ratio 355-358 F4.2 [-] e_[CeII/Fe] Error on [CeII/Fe] 360 I1 --- o_[CeII/Fe] ? Number of lines used to calculate [CeII/Fe] 362-365 F4.2 [-] [NdII/Fe] NdII to iron abundance ratio 367-370 F4.2 [-] e_[NdII/Fe] Error on [NdII/Fe] 372 I1 --- o_[NdII/Fe] ? Number of lines used to calculate [NdII/Fe] 374-377 F4.2 [-] [SmII/Fe] SmII to iron abundance ratio 379-382 F4.2 [-] e_[SmII/Fe] Error on [SmII/Fe] 384 I1 --- o_[SmII/Fe] ? Number of lines used to calculate [SmII/Fe] 386-389 F4.2 [-] [EuII/Fe] EuII to iron abundance ratio calculated by synthesis 391-394 F4.2 [-] e_[EuII/Fe] Error on [EuII/Fe] 396 I1 --- o_[EuII/Fe] ? Number of lines used to calculate [EuII/Fe] -------------------------------------------------------------------------------- Note (1): Flag as follows: * = We excluded the barium abundance of the star 310 in NGC 2168 in calculating the cluster mean [Ba/Fe] value due to the star's rapid rotation (Vrot∼12km/s) which may lead to turbulent superficial stellar layers from where the BaII lines emerge. As a result, the inclusion of microturbulence derived from Fe lines in the spectrum synthesis of a BaII line is insufficient to represent the true line broadening imposed by relatively turbulent upper photospheric layers on the BaII line, which may result in a serious overestimation of the Ba abundance by standard LTE abundance analysis (Reddy & Lambert 2017ApJ...845..151R 2017ApJ...845..151R). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table8.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Cluster Cluster name 10- 12 A3 --- Star Star ID (Avg stands for the average of the entire cluster) 14- 17 F4.2 [-] [NaI/Fe] NaI to iron abundance ratio 19- 22 F4.2 [-] e_[NaI/Fe] Error on [NaI/Fe] 24 I1 --- o_[NaI/Fe] ? Number of lines used to calculate [NaI/Fe] 26- 30 F5.2 [-] [MgI/Fe] MgI to iron abundance ratio 32- 35 F4.2 [-] e_[MgI/Fe] Error on [MgI/Fe] 37 I1 --- o_[MgI/Fe] ? Number of lines used to calculate [MgI/Fe] 39- 43 F5.2 [-] [AlI/Fe] AlI to iron abundance ratio 45- 48 F4.2 [-] e_[AlI/Fe] Error on [AlI/Fe] 50 I1 --- o_[AlI/Fe] ? Number of lines used to calculate [AlI/Fe] 52- 55 F4.2 [-] [SiI/Fe] SiI to iron abundance ratio 57- 60 F4.2 [-] e_[SiI/Fe] Error on [SiI/Fe] 62- 63 I2 --- o_[SiI/Fe] ? Number of lines used to calculate [SiI/Fe] 65- 68 F4.2 [-] [CaI/Fe] CaI to iron abundance ratio 70- 73 F4.2 [-] e_[CaI/Fe] Error on [CaI/Fe] 75- 76 I2 --- o_[CaI/Fe] ? Number of lines used to calculate [CaI/Fe] 78- 81 F4.2 [-] [ScI/Fe] ? ScI to iron abundance ratio 83- 86 F4.2 [-] e_[ScI/Fe] ? Error on [ScI/Fe] 88 I1 --- o_[ScI/Fe] ? Number of lines used to calculate [ScI/Fe] 90- 94 F5.2 [-] [ScII/Fe] ScII to iron abundance ratio 96- 99 F4.2 [-] e_[ScII/Fe] Error on [ScII/Fe] 101 I1 --- o_[ScII/Fe] ? Number of lines used to calculate [ScII/Fe] 103-106 F4.2 [-] [ScII/Fe]s ScII to iron abundance ratio calculated by synthesis 108-111 F4.2 [-] e_[ScII/Fe]s Error on [ScII/Fe]s 113 I1 --- o_[ScII/Fe]s ? Number of lines used to calculate [ScII/Fe]s 115-119 F5.2 [-] [TiI/Fe] TiI to iron abundance ratio 121-124 F4.2 [-] e_[TiI/Fe] Error on [TiI/Fe] 126-127 I2 --- o_[TiI/Fe] ? Number of lines used to calculate [TiI/Fe] 129-133 F5.2 [-] [TiII/Fe] TiII to iron abundance ratio 135-138 F4.2 [-] e_[TiII/Fe] Error on [TiII/Fe] 140-141 I2 --- o_[TiII/Fe] ? Number of lines used to calculate [TiII/Fe] 143-147 F5.2 [-] [VI/Fe] VI to iron abundance ratio 149-152 F4.2 [-] e_[VI/Fe] Error on [VI/Fe] 154-155 I2 --- o_[VI/Fe] ? Number of lines used to calculate [VI/Fe] 157-161 F5.2 [-] [CrI/Fe] CrI to iron abundance ratio 163-166 F4.2 [-] e_[CrI/Fe] Error on [CrI/Fe] 168-169 I2 --- o_[CrI/Fe] ? Number of lines used to calculate [CrI/Fe] 171-175 F5.2 [-] [CrII/Fe] CrII to iron abundance ratio 177-180 F4.2 [-] e_[CrII/Fe] Error on [CrII/Fe] 182 I1 --- o_[CrII/Fe] ? Number of lines used to calculate [CrII/Fe] 184-188 F5.2 [-] [MnI/Fe] MnI to iron abundance ratio calculated by synthesis 190-193 F4.2 [-] e_[MnI/Fe] Error on [MnI/Fe] 195 I1 --- o_[MnI/Fe] ? Number of lines used to calculate [MnI/Fe] 197-201 F5.2 [-] [FeI/H] FeI to hydrogen abundance ratio 203-206 F4.2 [-] e_[FeI/H] Error on [FeI/H] 208-210 I3 --- o_[FeI/H] ? Number of lines used to calculate [FeI/H] 212-216 F5.2 [-] [FeII/H] FeII to hydrogen abundance ratio 218-221 F4.2 [-] e_[FeII/H] Error on [FeII/H] 223-224 I2 --- o_[FeII/H] ? Number of lines used to calculate [FeII/H] 226-230 F5.2 [-] [CoI/Fe] CoI to iron abundance ratio 232-235 F4.2 [-] e_[CoI/Fe] Error on [CoI/Fe] 237 I1 --- o_[CoI/Fe] ? Number of lines used to calculate [CoI/Fe] 239-243 F5.2 [-] [NiI/Fe] NiI to iron abundance ratio 245-248 F4.2 [-] e_[NiI/Fe] Error on [NiI/Fe] 250-251 I2 --- o_[NiI/Fe] ? Number of lines used to calculate [NiI/Fe] 253-257 F5.2 [-] [CuI/Fe] CuI to iron abundance ratio calculated by synthesis 259-262 F4.2 [-] e_[CuI/Fe] Error on [CuI/Fe] 264 I1 --- o_[CuI/Fe] ? Number of lines used to calculate [CuI/Fe] 266-269 F4.2 [-] [ZnI/Fe] ZnI to iron abundance ratio calculated by synthesis 271-274 F4.2 [-] e_[ZnI/Fe] Error on [ZnI/Fe] 276 I1 --- o_[ZnI/Fe] ? Number of lines used to calculate [ZnI/Fe] 278-281 F4.2 [-] [YII/Fe] YII to iron abundance ratio 283-286 F4.2 [-] e_[YII/Fe] Error on [YII/Fe] 288-289 I2 --- o_[YII/Fe] ? Number of lines used to calculate [YII/Fe] 291-295 F5.3 [-] [ZrI/Fe] ZrI to iron abundance ratio 297-300 F4.2 [-] e_[ZrI/Fe] Error on [ZrI/Fe] 302 I1 --- o_[ZrI/Fe] ? Number of lines used to calculate [ZrI/Fe] 304-307 F4.2 [-] [ZrII/Fe] ZrII to iron abundance ratio 309-312 F4.2 [-] e_[ZrII/Fe] Error on [ZrII/Fe] 314 I1 --- o_[ZrII/Fe] ? Number of lines used to calculate [ZrII/Fe] 316-319 F4.2 [-] [BaII/Fe] BaII to iron abundance ratio calculated by synthesis 321-324 F4.2 [-] e_[BaII/Fe] Error on [BaII/Fe] 326 I1 --- o_[BaII/Fe] ? Number of lines used to calculate [BaII/Fe] 328-331 F4.2 [-] [LaII/Fe] LaII to iron abundance ratio 333-336 F4.2 [-] e_[LaII/Fe] Error on [LaII/Fe] 338 I1 --- o_[LaII/Fe] ? Number of lines used to calculate [LaII/Fe] 340-343 F4.2 [-] [CeII/Fe] CeII to iron abundance ratio 345-348 F4.2 [-] e_[CeII/Fe] Error on [CeII/Fe] 350 I1 --- o_[CeII/Fe] ? Number of lines used to calculate [CeII/Fe] 352-355 F4.2 [-] [NdII/Fe] NdII to iron abundance ratio 357-360 F4.2 [-] e_[NdII/Fe] Error on [NdII/Fe] 362-363 I2 --- o_[NdII/Fe] ? Number of lines used to calculate [NdII/Fe] 365-368 F4.2 [-] [SmII/Fe] SmII to iron abundance ratio 370-373 F4.2 [-] e_[SmII/Fe] Error on [SmII/Fe] 375 I1 --- o_[SmII/Fe] ? Number of lines used to calculate [SmII/Fe] 377-380 F4.2 [-] [EuII/Fe] ? EuII to iron abundance ratio calculated by synthesis 382-385 F4.2 [-] e_[EuII/Fe] ? Error on [EuII/Fe] 387 I1 --- o_[EuII/Fe] ? Number of lines used to calculate [EuII/Fe] -------------------------------------------------------------------------------- Byte-by-byte Description of file: table9.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Cluster Cluster name 10- 12 A3 --- Star Star ID (Avg stands for the average of the entire cluster) 14- 17 F4.2 [-] [NaI/Fe] NaI to iron abundance ratio 19- 22 F4.2 [-] e_[NaI/Fe] Error on [NaI/Fe] 24 I1 --- o_[NaI/Fe] ? Number of lines used to calculate [NaI/Fe] 26- 29 F4.2 [-] [MgI/Fe] MgI to iron abundance ratio 31- 34 F4.2 [-] e_[MgI/Fe] Error on [MgI/Fe] 36 I1 --- o_[MgI/Fe] ? Number of lines used to calculate [MgI/Fe] 38- 41 F4.2 [-] [AlI/Fe] AlI to iron abundance ratio 43- 46 F4.2 [-] e_[AlI/Fe] Error on [AlI/Fe] 48 I1 --- o_[AlI/Fe] ? Number of lines used to calculate [AlI/Fe] 50- 53 F4.2 [-] [SiI/Fe] SiI to iron abundance ratio 55- 58 F4.2 [-] e_[SiI/Fe] Error on [SiI/Fe] 60- 61 I2 --- o_[SiI/Fe] ? Number of lines used to calculate [SiI/Fe] 63- 67 F5.2 [-] [CaI/Fe] CaI to iron abundance ratio 69- 72 F4.2 [-] e_[CaI/Fe] Error on [CaI/Fe] 74- 75 I2 --- o_[CaI/Fe] ? Number of lines used to calculate [CaI/Fe] 77- 81 F5.2 [-] [ScII/Fe] ScII to iron abundance ratio 83- 86 F4.2 [-] e_[ScII/Fe] Error on [ScII/Fe]] 88 I1 --- o_[ScII/Fe] ? Number of lines used to calculate [ScII/Fe] 90- 93 F4.2 [-] [ScII/Fe]s ScII to iron abundance ratio calculated by synthesis 95- 98 F4.2 [-] e_[ScII/Fe]s Error on [ScII/Fe]s 100 I1 --- o_[ScII/Fe]s ? Number of lines used to calculate [ScII/Fe]s 102-106 F5.2 [-] [TiI/Fe] TiI to iron abundance ratio 108-111 F4.2 [-] e_[TiI/Fe] Error on [TiI/Fe] 113-114 I2 --- o_[TiI/Fe] ? Number of lines used to calculate [TiI/Fe] 116-120 F5.2 [-] [TiII/Fe] TiII to iron abundance ratio 122-125 F4.2 [-] e_[TiII/Fe] Error on [TiII/Fe] 127 I1 --- o_[TiII/Fe] ? Number of lines used to calculate [TiII/Fe] 129-132 F4.2 [-] [VI/Fe] VI to iron abundance ratio 134-137 F4.2 [-] e_[VI/Fe] Error on [VI/Fe] 139-140 I2 --- o_[VI/Fe] ? Number of lines used to calculate [VI/Fe] 142-146 F5.2 [-] [CrI/Fe] CrI to iron abundance ratio 148-151 F4.2 [-] e_[CrI/Fe] Error on [CrI/Fe] 153-154 I2 --- o_[CrI/Fe] ? Number of lines used to calculate [CrI/Fe] 156-159 F4.2 [-] [CrII/Fe] CrII to iron abundance ratio 161-164 F4.2 [-] e_[CrII/Fe] Error on [CrII/Fe] 166 I1 --- o_[CrII/Fe] ? Number of lines used to calculate [CrII/Fe] 168-172 F5.2 [-] [MnI/Fe] MnI to iron abundance ratio calculated by synthesis 174-177 F4.2 [-] e_[MnI/Fe] Error on [MnI/Fe] 179 I1 --- o_[MnI/Fe] ? Number of lines used to calculate [MnI/Fe] 181-185 F5.2 [-] [FeI/H] FeI to hydrogen abundance ratio 187-190 F4.2 [-] e_[FeI/H] Error on [FeI/H] 192-194 I3 --- o_[FeI/H] ? Number of lines used to calculate [FeI/H] 196-200 F5.2 [-] [FeII/H] FeII to hydrogen abundance ratio 202-205 F4.2 [-] e_[FeII/H] Error on [FeII/H] 207-208 I2 --- o_[FeII/H] ? Number of lines used to calculate [FeII/H] 210-213 F4.2 [-] [CoI/Fe] CoI to iron abundance ratio 215-218 F4.2 [-] e_[CoI/Fe] Error on [CoI/Fe] 220 I1 --- o_[CoI/Fe] ? Number of lines used to calculate [CoI/Fe] 222-226 F5.2 [-] [NiI/Fe] NiI to iron abundance ratio 228-231 F4.2 [-] e_[NiI/Fe] Error on [NiI/Fe] 233-234 I2 --- o_[NiI/Fe] ? Number of lines used to calculate [NiI/Fe] 236-239 F4.2 [-] [CuI/Fe] CuI to iron abundance ratio calculated by synthesis 241-244 F4.2 [-] e_[CuI/Fe] Error on [CuI/Fe] 246 I1 --- o_[CuI/Fe] ? Number of lines used to calculate [CuI/Fe] 248-252 F5.2 [-] [ZnI/Fe] ZnI to iron abundance ratio calculated by synthesis 254-257 F4.2 [-] e_[ZnI/Fe] Error on [ZnI/Fe] 259 I1 --- o_[ZnI/Fe] ? Number of lines used to calculate [ZnI/Fe] 261-264 F4.2 [-] [YII/Fe] YII to iron abundance ratio 266-269 F4.2 [-] e_[YII/Fe] Error on [YII/Fe] 271 I1 --- o_[YII/Fe] ? Number of lines used to calculate [YII/Fe] 273-277 F5.2 [-] [ZrI/Fe] ZrI to iron abundance ratio 279-282 F4.2 [-] e_[ZrI/Fe] Error on [ZrI/Fe] 284 I1 --- o_[ZrI/Fe] ? Number of lines used to calculate [ZrI/Fe] 286-290 F5.2 [-] [ZrII/Fe] ZrII to iron abundance ratio 292-295 F4.2 [-] e_[ZrII/Fe] Error on [ZrII/Fe] 297 I1 --- o_[ZrII/Fe] ? Number of lines used to calculate [ZrII/Fe] 299-302 F4.2 [-] [BaII/Fe] BaII to iron abundance ratio calculated by synthesis 304-307 F4.2 [-] e_[BaII/Fe] Error on [BaII/Fe] 309 I1 --- o_[BaII/Fe] ? Number of lines used to calculate [BaII/Fe] 311-314 F4.2 [-] [LaII/Fe] LaII to iron abundance ratio 316-319 F4.2 [-] e_[LaII/Fe] Error on [LaII/Fe] 321 I1 --- o_[LaII/Fe] ? Number of lines used to calculate [LaII/Fe] 323-326 F4.2 [-] [CeII/Fe] CeII to iron abundance ratio 328-331 F4.2 [-] e_[CeII/Fe] Error on [CeII/Fe] 333 I1 --- o_[CeII/Fe] ? Number of lines used to calculate [CeII/Fe] 335-338 F4.2 [-] [NdII/Fe] NdII to iron abundance ratio 340-343 F4.2 [-] e_[NdII/Fe] Error on [NdII/Fe] 345 I1 --- o_[NdII/Fe] ? Number of lines used to calculate [NdII/Fe] 347-350 F4.2 [-] [SmII/Fe] SmII to iron abundance ratio 352-355 F4.2 [-] e_[SmII/Fe] Error on [SmII/Fe] 357 I1 --- o_[SmII/Fe] ? Number of lines used to calculate [SmII/Fe] 359-362 F4.2 [-] [EuII/Fe] EuII to iron abundance ratio calculated by synthesis 364-367 F4.2 [-] e_[EuII/Fe] Error on [EuII/Fe] 369 I1 --- o_[EuII/Fe] ? Number of lines used to calculate [EuII/Fe] -------------------------------------------------------------------------------- Byte-by-byte Description of file: table10.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Cluster Cluster name 10- 14 F5.2 [-] [Fe/H] Iron to hydrogen abundance ratio 16- 19 F4.2 [-] e_[Fe/H] Error on [Fe/H] 21- 24 F4.2 [-] [Na/Fe]LTE Mean LTE Na to Fe abundance ratio 26- 29 F4.2 [-] e_[Na/Fe]LTE Error on [Na/Fe]LTE 31- 34 F4.2 [-] [Na/Fe] Mean non-LTE Na to Fe abundance ratio (1) 36- 39 F4.2 [-] e_[Na/Fe] Error on [Na/Fe] 41- 45 F5.2 [-] [Al/Fe]LTE Mean LTE Al to Fe abundance ratio 47- 50 F4.2 [-] e_[Al/Fe]LTE Error on [Al/Fe]LTE 52- 56 F5.2 [-] [Al/Fe] Mean non-LTE Al to Fe abundance ratio (2) 58- 61 F4.2 [-] e_[Al/Fe] Error on [Al/Fe] 63- 66 F4.2 Msun Mturnoff Cluster's turn-off mass -------------------------------------------------------------------------------- Note (1): For all giants in this and earlier papers in this series, the Na abundances derived assuming LTE were corrected for non-LTE effects using the grids of Lind et al. (2011A&A...528A.103L 2011A&A...528A.103L). The corrections were derived on a line-by-line basis, using the stellar parameters (Teff, logg) and the EWs of Na lines (5688.20, 6154.22, and 6160.74Å) of each star as input to the interactive non-LTE data base. Note (2): The non-LTE corrections for Al were computed using the extensive grids of abundance corrections discussed in Nordlander & Lind (2017A&A...607A..75N 2017A&A...607A..75N). The non-LTE Al abundance calculations were carried out using the stellar parameters and LTE Al abundances for the 7835, 7836, 8773, and 8774Å lines as input to the source code of Nordlander & Lind (2017A&A...607A..75N 2017A&A...607A..75N). -------------------------------------------------------------------------------- History: From electronic version of the journal References: Reddy et al., Paper I 2012MNRAS.419.1350R 2012MNRAS.419.1350R, Cat. J/MNRAS/419/1350 Reddy et al., Paper II 2013MNRAS.431.3338R 2013MNRAS.431.3338R, Cat. J/MNRAS/431/3338 Reddy et al., Paper III 2015MNRAS.450.4301R 2015MNRAS.450.4301R, Cat. J/MNRAS/450/4301 Reddy et al., Paper IV 2016MNRAS.463.4366R 2016MNRAS.463.4366R
(End) Ana Fiallos [CDS] 23-Sep-2022
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line